Protoplanetary disk chemistry
KI Öberg, S Facchini… - Annual Review of …, 2023 - annualreviews.org
Planets form in disks of gas and dust around young stars. The disk molecular reservoirs and
their chemical evolution affect all aspects of planet formation, from the coagulation of dust …
their chemical evolution affect all aspects of planet formation, from the coagulation of dust …
Molecules with ALMA at Planet-forming Scales (MAPS). I. Program overview and highlights
Planets form and obtain their compositions in dust-and gas-rich disks around young stars,
and the outcome of this process is intimately linked to the disk chemical properties. The …
and the outcome of this process is intimately linked to the disk chemical properties. The …
The disk substructures at high angular resolution project (DSHARP). I. Motivation, sample, calibration, and overview
Abstract We introduce the Disk Substructures at High Angular Resolution Project (DSHARP),
one of the initial Large Programs conducted with the Atacama Large Millimeter/submillimeter …
one of the initial Large Programs conducted with the Atacama Large Millimeter/submillimeter …
Disks around t tauri stars with sphere (dartts-s). i. sphere/irdis polarimetric imaging of eight prominent t tauri disks
We present the first part of our Disks ARound T Tauri Stars with SPHERE (DARTTS-S)
survey: observations of eight T Tauri stars that were selected based on their strong (sub) …
survey: observations of eight T Tauri stars that were selected based on their strong (sub) …
A kinematical detection of two embedded Jupiter-mass planets in HD 163296
We present the first kinematical detection of embedded protoplanets within a protoplanetary
disk. Using archival Atacama Large Millimetre Array (ALMA) observations of HD 163296, we …
disk. Using archival Atacama Large Millimetre Array (ALMA) observations of HD 163296, we …
Molecules with ALMA at planet-forming scales (MAPS). III. Characteristics of radial chemical substructures
The Molecules with ALMA at Planet-forming Scales (MAPS) Large Program provides a
detailed, high-resolution (∼ 10–20 au) view of molecular line emission in five protoplanetary …
detailed, high-resolution (∼ 10–20 au) view of molecular line emission in five protoplanetary …
Measuring turbulent motion in planet-forming disks with ALMA: a detection around DM Tau and nondetections around MWC 480 and V4046 Sgr
Turbulence is a crucial factor in many models of planet formation, but it has only been
directly constrained among a small number of planet-forming disks. Building on the upper …
directly constrained among a small number of planet-forming disks. Building on the upper …
A three-dimensional view of turbulence: constraints on turbulent motions in the HD 163296 protoplanetary disk using DCO+
KM Flaherty, AM Hughes, SC Rose… - The Astrophysical …, 2017 - iopscience.iop.org
Gas kinematics are an important part of the planet formation process. Turbulence influences
planetesimal growth and migration from the scale of submicron dust grains through gas …
planetesimal growth and migration from the scale of submicron dust grains through gas …
A millimeter Continuum Size–Luminosity Relationship for Protoplanetary Disks
We present a survey at subarcsecond resolution of the 340 GHz dust continuum emission
from 50 nearby protoplanetary disks, based on new and archival observations with the …
from 50 nearby protoplanetary disks, based on new and archival observations with the …
Direct mapping of the temperature and velocity gradients in discs-Imaging the vertical CO snow line around IM Lupi
Accurate measurements of the physical structure of protoplanetary discs are critical inputs
for planet formation models. These constraints are traditionally established via complex …
for planet formation models. These constraints are traditionally established via complex …